Draconids 2011: Outburst Observations by the Croatian Meteor Network |
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Authors: | Damir Šegon Željko Andreić Peter S. Gural Korado Korlević Denis Vida Filip Novoselnik Ivica Skokić |
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Affiliation: | 1. Astronomical Society “Istra” Pula, Park Monte Zaro 2, 52100, Pula, Croatia 2. Vi?njan Science and Education Center, Istarska 5, 51463, Vi?njan, Croatia 3. Faculty of Mining, Geology and Petroleum Engineering, University of Zagreb, Pierottijeva 6, 10000, Zagreb, Croatia 4. 351 Samantha Drive, Sterling, VA, 20164, USA 5. Astronomical Society Anonymus, B. Radi?a 34, 31550, Valpovo, Croatia 6. Faculty of Electrical Engineering, University of Osijek, Kneza Trpimira 2B, 31000, Osijek, Croatia
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Abstract: | The predicted Draconid meteor shower outburst during October 2011 had been observed by a portion of the Croatian Meteor Network whose stations encountered clear weather. A total of 95 Draconid orbits have been calculated from 18 contributing stations, and in this paper we present results for 63 orbits obtained from the fully automatic observation and processing pipeline. Two methods of trajectory estimation were applied, showing better fit results using a linearly changing velocity model versus a constant velocity model. The estimated mean radiant position has been found to be at RA = 262.6°, Dec = +55.7°, with estimated geocentric velocity Vg = 20.7 km/s. |
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